Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

Dra̧żkowska, Joanna; Li, Shengtai; Birnstiel, Til; Stammler, Sebastian M.; Li, Hui

doi:10.3847/1538-4357/ab46b7

Title: Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

Journal Article · Fri Nov 01 00:00:00 EDT 2019 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/ab46b7· OSTI ID:1764231

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Ludwig Maximillian Univ. of Munich (Germany). University Observatory
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

Dust growth is often neglected when building models of protoplanetary disks due to its complexity and computational expense. However, it does play a major role in shaping the evolution of protoplanetary dust and planet formation. In this paper, we present a numerical model coupling 2D hydrodynamic evolution of a protoplanetary disk, including a Jupiter-mass planet, and dust coagulation. This is obtained by including multiple dust fluids in a single grid-based hydrodynamic simulation and solving the Smoluchowski equation for dust coagulation on top of solving for the hydrodynamic evolution. We find that fragmentation of dust aggregates trapped in a pressure bump outside of the planetary gap leads to an enhancement in the density of small grains. Additionally, we compare the results obtained from the full-coagulation treatment to the commonly used, fixed-dust-size approach and to previously applied, less computationally intensive methods for including dust coagulation. We find that the full-coagulation results cannot be reproduced using the fixed-size treatment, but some can be mimicked using a relatively simple method for estimating the characteristic dust size in every grid cell.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA); European Research Council (ERC); National Science Foundation (NSF)

Grant/Contract Number:: 89233218CNA000001; 714769; PHY-1607611

OSTI ID:: 1764231

Report Number(s):: LA-UR-20-28594; TRN: US2206158

Journal Information:: The Astrophysical Journal (Online), Vol. 885, Issue 1; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Li, Ya-Ping; Li, Hui; Li, Shengtai; +3 more

ELECTROSTATIC BARRIER AGAINST DUST GROWTH IN PROTOPLANETARY DISKS. I. CLASSIFYING THE EVOLUTION OF SIZE DISTRIBUTION

Journal Article · Wed Apr 20 00:00:00 EDT 2011 · Astrophysical Journal · OSTI ID:1764231

Okuzumi, Satoshi; Sakagami, Masa-aki; Tanaka, Hidekazu; +1 more

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79 ASTRONOMY AND ASTROPHYSICS
accretion
accretion disks
numerical methods
planets and satellites
protoplanetary disks
planet-disk interactions

Title: Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

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